EXAM II Study Flashcards

1
Q

What is the main purpose of a telescope

A

To collect as much light as possible in the shortest time and resolve small details

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2
Q

What determines a telescope’s efficiency

A

The area of the mirror or lens

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3
Q

Why are the large mirrors preferred over lenses for telescopes

A

they are cheaper, easier to maintain, and suffer less from absorption and refraction

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4
Q

what are the main uses of telescopes

A

imaging, spectroscopic studies, and long term monitoring

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5
Q

what limits ground-based telescopes

A

atmospheric distortion, which can be improved by adaptive optics and interferometry

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6
Q

what are the three main types of spectra

A

continuous, discrete, and absorption

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7
Q

continuous spectra

A

When light emitted from a solid substance passes through a prism, it produces a continuous spectrum of colors

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8
Q

emission spectra

A

a spectrum of the electromagnetic radiation emitted by a source.

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9
Q

absorption spectra

A

A combination of emission and continuous spectra

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10
Q

what kinds of material produces a continuous spectrum

A

hot, dense materials like solids. Spectral lines are unique to the element that produced them, making them identifiers of elements which can be used to identify elements in the composition of distant astrophysical objects

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11
Q

what produces an absorption spectrum

A

a cold gas in front of a hot source, absorbing specific wavelengths. the dark lines are emission lines that have been absorbed. These emission lines correspond to energy levels in atoms.

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12
Q

how are spectral lines used in astronomy

A

to identify elements and determine velocity and direction via the Doppler effect

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13
Q

what are the main components of the sun

A

hydrogen and helium

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14
Q

what percentage of the sun is hydrogen

A

more than 70%

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15
Q

what percentage of the sun is helium

A

more than 20%

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16
Q

What are the three main layers of the sun

A

core, radiative zone, and convective zone

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17
Q

How does energy move within the sun?

A

photon diffusion in the radiative zone, conviction in the convective zone

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18
Q

what is the solar wind?

A

a stream of charged particles escaping the sun

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19
Q

How is the sun’s magnetic field generated

A

by differential rotation of plasma layers

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20
Q

what defines a star?

A

an object that produces energy via nuclear fusion

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21
Q

what are the two main types of planets

A

jovian and terrestrial

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22
Q

what differentiates dwarf planets from other planets

A

they are small, icy/rocky, and do not clear the orbits

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23
Q

what are asteroids

A

irregularly shaped rocky/metallic objects mostly found in the asteroid belt

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24
Q

what are the primary characteristics of jovian planets

A

large, gas-rich, possesses rings, and many moons, strong magnetic fields

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25
Q

why is venus the hottest planet

A

its dense CO2 atmosphere creates a strong greenhouse effect

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26
Q

what evidence suggests mars once had liquid water?

A

surface features indicating past water flow

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27
Q

what is unique about uranus and venus’ rotation?

A

they rotate in a different direction than other planets

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28
Q

what is the great red spot on jupiter

A

a massive storm that has lasted for centuries

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29
Q

why does jupiter emit more energy than it recieves?

A

due to gravitational contraction and internal heating

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30
Q

what is gravitational contraction

A

the process in which gravity causes an object to contract, thereby converting gravitational potential energy into thermal energy

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31
Q

doppler effect

A

An observed change in the frequency of a wave when the source or observer is moving

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32
Q

What is the surface temperature of the sun

A

5700 degrees K

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33
Q

How hot is the core temperature of the sun

A

15 million degrees Celsius (27 million degrees Fahrenheit), hot enough to sustain nuclear fusion

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34
Q

How long does the journey take for the energy from the core to reach the sun’s surface

A

100,000 years

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35
Q

What are the two forces that keep the sun in a constant state of equilibrium

A

gravitation and radiation pressure

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36
Q

The Sun converts hydrogen to helium in its ______.

A

core, via nuclear fusion

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37
Q

What is the prime reaction in the proton-proton chain where nuclear fusion occurs

A

4 protons are converted to helium, energy, positrons, and neutrinos

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38
Q

High temperature is needed in the sun to overcome what?

A

core, repulsive electromagnetic force due to positive, proton-proton, nuclei

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39
Q

Why is the very high density in the core needed

A

to accommodate interactions between protons

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40
Q

Nuclear reactions in the core generate vast amounts of ___ which is transported through the ___ zone via ____

A

energy, radiative zone, photon difussion

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41
Q

what is proton difussion

A

scattering and absorption

42
Q

How is energy transported in the convective zone

A

via physical motion of hydrogen gas/plasma

43
Q

Outer layers of the sun include a ___ which we see as a surface

A

photosphere

44
Q

how deep is the photosphere

A

thin, a few hundred kms

45
Q

what is the corona

A

a wispy layer of the sun approximately 1 million degrees and is only seen when the central disk of the sun is blocked

46
Q

why is the corona very hot

A

energetic electrons moving under the action of magnetic field

47
Q

what is the solar wind comprised of

A

energetic electrons, protons, and helium ions which escape the surface and travel outwards, interacting with objects in the solar system

48
Q

How do we know the structure of the interior of the sun?

A

modeling motion of gas/plasma using the laws of physics and via measuring properties of escaped particles such as neutrinos, electrons, positrons, protons, helium ions etc.

49
Q

How do we know the temperature of the surface of the Sun?

A

measuring the continuous spectrum of the sun

50
Q

How do we know the constituents of the Sun

A

by analyzing the spectral lines, hydrogen and helium emission lines

51
Q

the sun has a magnetic field, how is it generated ?

A

via the differential rotation of gasses/plasma layers that include moving charges

52
Q

What is nuclear fusion, in terms of the star

A

the proton-proton chain that produces He and energy, which is the simplest reaction

53
Q

at what temperature does the p-p chain of He and energy occur

A

between 10 and 15 million degrees kelvin

54
Q

at what rate does the sun rotate about its axis?

A

1 revolution per 27 days

55
Q

how hot is the sun’s surface temperature

A

around 6,000 degrees K

56
Q

what is the sun’s magnetic field comprised of

A

a Hydrogen and Helium mixture where Hydrogen dominates at around 70%

57
Q

What are the characteristics of our solar system’s behavior

A

all planets revolve around the sun in the same direction and in a similar plane. all planets rotate about their own axis

58
Q

What shape are the majority of the orbits in the solar system

A

elliptical

59
Q

What are characteristics of mercury

A
  • extreme variation between day/night temperatures
60
Q
  • no atmosphere
61
Q
  • small magnetic field
62
Q
  • heavily cratered, likely due to collisions during its formation
63
Q

What are characteristics of venus

A
  • hottest planet because of greenhouse effect
64
Q

What are characteristics of Mars

A
  • light atmosphere of CO2
65
Q
  • possesses a magnetic field
66
Q
  • surface features indicate flow of water
67
Q
  • has 2 irregular shaped moons, probably captured asteroids
68
Q

What is the most dominant jovian planet?

69
Q

What is Jupiter comprised of

A

Hydrogen and Helium, though not massive enough to produce nuclear fusion

70
Q

Why does jupiter produce a large magnetic field

A

electrical charges moving in the interior as well as a differential rotation of the surface layers. At the deepest layer, hydrogen behaves like a liquid metal

71
Q

We know how fast a distant galaxy is moving away from us on the basis of its

A

spectrum, doppler effect

72
Q

According to the laws of thermal radiation, hotter objects emit photons with

A

a shorter average wavelength

73
Q

Suppose you know the frequency of a photon and the speed of light. What else can you determine about the photon?

A

its wavelength and energy

74
Q

We can see the Moon because it

A

reflects visible light

75
Q

You observe a distant galaxy. You find that a spectral line of hydrogen that is shifted from its normal location in the visible part of the spectrum into the infrared part of the spectrum. What can you conclude?

A

the galaxy is moving away from you

76
Q

Which of the following conditions lead you to see an absorption line spectrum from a cloud of gas in interstellar space?

A

The cloud is cool and lies between you and a hot star

77
Q

From shortest to longest wavelength, which of the following correctly orders the different categories of electromagnetic radiation?

A

gamma rays, x-rays, ultraviolet, visible light, infrared, radio

78
Q

Suppose you want to know the chemical composition of a distant star. Which piece of information is most useful to you?

A

the wavelengths of spectral lines in the star’s spectrum

79
Q

Laboratory measurements show hydrogen produces a spectral line at a wavelength of 486.1 nanometers (nm). A particular star’s spectrum shows the same hydrogen line at a wavelength of 486.0 nm. What can we conclude?

A

The star is moving toward us.

80
Q

Thermal radiation is defined as

A

radiation with a spectrum whose shape depends only on the temperature of the emitting object.

81
Q

Suppose that Star X and Star Y both have redshifts, but Star X has a larger redshift than Star Y. What can you conclude?

A

Star X is moving away from us faster than Star Y

82
Q

Betelgeuse is the bright red star representing the left shoulder of the constellation Orion. All the following statements about Betelgeuse are true. Which one can you infer from its red color?

A

Its surface is cooler than the surface of the Sun.

83
Q

Which of the following stars is the hottest? Red star, yellow star, blue star, green star

84
Q

What observational techniques is most appropriate for measuring Doppler shifts?

A

spectroscopy

85
Q

Suppose that two stars are identical in every way; for example, same distance, same mass, same temperature, same chemical composition, and same speed relative to Earth, except that one star rotates faster than the other. Spectroscopically, how could you tell the stars apart?

A

The faster rotating star has wider spectral lines than the slower rotating star.

86
Q

When an atom’s electrons fall down to lower energy levels in a thin cloud of hot gas, what is produced?

A

an emission line spectrum

87
Q

We know the Sun is primarily made from hydrogen and helium on the basis of its

88
Q

The Chandra X-ray Observatory must operate in space because

A

x-rays do not penetrate Earth’s atmosphere

89
Q

Which of the following observational techniques is most appropriate for measuring Doppler shifts?

A

spectroscopy

90
Q

What telescope is best suited for studying the hottest intergalactic gas (10 million K) in a cluster of galaxies?

A

Chandra X-ray Telescope

91
Q

Why can’t x-ray and gamma-ray telescopes use the same designs as visible-light telescopes?

A

X-rays and gamma rays have so much energy that they cannot be reflected in the same way as visible light.

92
Q

What is the purpose of interferometry?

A

It allows two or more small telescopes to achieve the angular resolution of a much larger telescope.

93
Q

What does angular resolution measure?

A

the angular size of the smallest features that the telescope can see

94
Q

What is the purpose of adaptive optics?

A

It reduces blurring caused by atmospheric turbulence for telescopes on the ground.

95
Q

The stars in our sky twinkle in brightness and color because of

A

turbulence in the Earth’s atmosphere.

96
Q

Which of the following wavelength regions can be studied with telescopes on the ground?

A

radio, visible, and very limited portions of the infrared and ultraviolet regions

97
Q

The light-collecting area of an 8-meter telescope is ________ times that of a 2-meter telescope.

98
Q

Which of the following best describes why radio telescopes are generally much larger in size than telescopes designed to collect visible light?

A

Getting an image of the same angular resolution requires a much larger telescope for radio waves than for visible light.

99
Q

Which of the following statements best describes the difference between a refracting telescope and a reflecting telescope?

A

A refracting telescope uses a transparent glass lens to focus light, whereas a reflecting telescope uses a mirror to focus light.

100
Q

Suppose you want to determine the chemical composition of a distant planet or star. Which of the following will be most useful to have?

A

high spectral resolution